Precision studies of cosmic rays with the PAMELA satellite experiment
2009 (English)In: 2009 IEEE NUCLEAR SCIENCE SYMPOSIUM CONFERENCE RECORD, VOLS 1-5 / [ed] Yu, B, IEEE , 2009, 2125-2130 p.Conference paper (Refereed)
The PAMELA satellite experiment was launched into low earth orbit on June 15th 2006. The combination of a permanent magnet silicon strip spectrometer, and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV - 200 GeV). A primary scientific goal is to search for dark matter particle annihilations by measuring the energy spectra of cosmic ray antiparticles. Latest results from the PAMELA experiment will be reviewed with a particular focus on cosmic ray antiprotons and positrons. The status of PAMELA measurements for other cosmic ray species will also be reviewed.
Place, publisher, year, edition, pages
IEEE , 2009. 2125-2130 p.
, IEEE Nuclear Science Symposium Conference Record, ISSN 1082-3654
Astronomy, Astrophysics and Cosmology
IdentifiersURN: urn:nbn:se:kth:diva-80117DOI: 10.1109/NSSMIC.2009.5402107ISI: 000280505101097ScopusID: 2-s2.0-77951174063ISBN: 978-142443962-1OAI: oai:DiVA.org:kth-80117DiVA: diva2:496016
2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009; Orlando, FL; 25 October 2009 through 31 October 2009
QC 201203092012-02-092012-02-092012-03-09Bibliographically approved